Migration-driven Planet Growth
Migration-Driven Planet Growth is a theoretical framework in planetary formation that explains the enhancement of planetary core accretion and final mass distribution through the inward or outward orbital migration of protoplanetary embryos, distinguishing it from static in-situ growth models by incorporating dynamical migration effects as a central mechanism for planet assembly.
52
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5.1K
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74
Authors
71
Institutions
Publications per year
2017–2026
24
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52
A low mass for Mars from Jupiter’s early gas-driven migration
K. J. Walsh, Alessandro Morbidelli, Sean N. Raymond et al. · Nature · 2011 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +16
Models of giant planet formation with migration and disc evolution
Y. Alibert, C. Mordasini, W. Benz et al. · Astronomy and Astrophysics · 2005 · 694 citations · Full text
Natural Sciences, Astronomy, Physics +15
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Centre National de la Recherche Scientifique
Paris, France
10 h-index
16 publications
4.7K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
10 h-index
15 publications
721 citations
Université de Bordeaux
Bordeaux, France
7 h-index
8 publications
1.8K citations
Laboratoire d'Astrophysique de Bordeaux
Bordeaux, France
7 h-index
8 publications
1.8K citations
University of Bern
Bern, Switzerland
6 h-index
20 publications
3.2K citations
Universidade Estadual Paulista (Unesp)
São Paulo, Brazil
6 h-index
8 publications
663 citations

Lund University
Lund, Sweden
5 h-index
7 publications
711 citations
Observatoire de la Côte d’Azur
Nice, France
5 h-index
6 publications
2.6K citations
1–8 of 71
12 publications · 1.4K citations
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10 publications · 571 citations
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6 publications · 338 citations
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ApJ · 5 publications · 307 citations
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Repository · 5 publications · 234 citations
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